The Physics of Cosmology
Autor Fulvio Meliaen Limba Engleză Paperback – apr 2026
Covering a wide range of topics from the Early Universe to the Semi-Classical Universe, this book stands out for its clarity and breadth, making it a valuable resource for students and researchers in general relativity and astrophysics. The book not only highlights the leading contributors and pivotal discoveries in the field but also provides timely and original material that supports both learning and instruction, keeping pace with cosmology’s rapid evolution over the past decade.
- Demonstrates the close linkage between cosmology and fundamental branches in physics, including general relativity, quantum mechanics, particle physics, and statistical mechanics.
- Moves seamlessly between theory and data interpretation.
- Offers a direct, foundational approach to the content, supported by pedagogical features including extensive end-of-chapter key term definitions.
- Showcases numerous illustrations, diagrams, and figures that provide visual clarity to the cosmological topics at hand.
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Specificații
ISBN-13: 9780443452017
ISBN-10: 0443452016
Pagini: 504
Dimensiuni: 191 x 235 mm
Editura: ELSEVIER SCIENCE
ISBN-10: 0443452016
Pagini: 504
Dimensiuni: 191 x 235 mm
Editura: ELSEVIER SCIENCE
Cuprins
Table of Contents
Preface
Dedication
1. An Inevitable Transition
2. The Friedmann-Lemaitre-Robertson-Walker Metric
3. The R{sub|h} = ct Universe
4. A Non-Inflated Expansion
5. The Primordial Power Spectrum
6. The Early Universe
7. The Semi-Classical Universe I
8. The Semi-Classical Universe II
9. Cosmic Microwave Background
10. Observational Tests at Low Redshift
11. Impact on Fundamental Physics
12. Future Developments
Preface
Dedication
1. An Inevitable Transition
2. The Friedmann-Lemaitre-Robertson-Walker Metric
3. The R{sub|h} = ct Universe
4. A Non-Inflated Expansion
5. The Primordial Power Spectrum
6. The Early Universe
7. The Semi-Classical Universe I
8. The Semi-Classical Universe II
9. Cosmic Microwave Background
10. Observational Tests at Low Redshift
11. Impact on Fundamental Physics
12. Future Developments